2017
DOI: 10.5194/gmd-10-4723-2017
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<sup>231</sup>Pa and <sup>230</sup>Th in the ocean model of the Community Earth System Model (CESM1.3)

Abstract: Abstract. The sediment 231 Pa / 230 Th activity ratio is emerging as an important proxy for deep ocean circulation in the past. In order to allow for a direct model-data comparison and to improve our understanding of the sediment 231 Pa / 230 Th activity ratio, we implement 231 Pa and 230 Th in the ocean component of the Community Earth System Model (CESM). In addition to the fully coupled implementation of the scavenging behavior of 231 Pa and 230 Th with the active marine ecosystem module (particle-coupled: … Show more

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Cited by 23 publications
(38 citation statements)
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References 108 publications
(116 reference statements)
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“…However, by comparing results from the p ‐coupled and p ‐fixed Nd setups, we find that the ε Nd changes in our model are mainly controlled by the circulation change. This is different from 231 Pa/ 230 Th in the CESM, which was found to be controlled by both the circulation and the productivity of biogenic particles (Gu & Liu, ). The changes in ε Nd caused by changes in biological productivity are much smaller than the ε Nd changes caused by changes in the circulation (Figures c, f, and g).…”
Section: Resultsmentioning
confidence: 72%
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“…However, by comparing results from the p ‐coupled and p ‐fixed Nd setups, we find that the ε Nd changes in our model are mainly controlled by the circulation change. This is different from 231 Pa/ 230 Th in the CESM, which was found to be controlled by both the circulation and the productivity of biogenic particles (Gu & Liu, ). The changes in ε Nd caused by changes in biological productivity are much smaller than the ε Nd changes caused by changes in the circulation (Figures c, f, and g).…”
Section: Resultsmentioning
confidence: 72%
“…In HOSING, the productivity of CaCO 3 , opal, and POC in the North Atlantic is greatly reduced (Gu & Liu, ) because of reduced nutrient supply resulting from the increase of stratification (Plattner et al, ; Schmittner, ). The resulting particle flux changes could also lead to a change in the p ‐coupled ε Nd (Rempfer et al, ).…”
Section: Resultsmentioning
confidence: 99%
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